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Related papers: An Extremely Bright QSO at $z=2.89$

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We report the discovery of the ultra-luminous QSO SMSS~J215728.21-360215.1 with magnitude $z=16.9$ and W4$=7.42$ at redshift 4.75. Given absolute magnitudes of $M_{145,\rm AB}=-29.3$, $M_{300,\rm AB}=-30.12$ and $\log L_{\rm bol}/L_{\rm…

We report the discovery of a bright (g = 14.5 mag (AB), K = 11.9 mag (Vega)) quasar at redshift z = 0.83 -- the optically brightest (unbeamed) quasar at z > 0.4. SMSS J114447.77-430859.3, at a Galactic latitude of b = +18.1deg, was…

We search for ultra-luminous Quasi-Stellar Objects (QSOs) at high redshift using photometry from the SkyMapper Southern Survey Data Release 3 (DR3), in combination with 2MASS, VHS DR6, VIKING DR5, AllWISE, and CatWISE2020, as well as…

Cosmology and Nongalactic Astrophysics · Physics 2022-01-19 Christopher A. Onken , Christian Wolf , Fuyan Bian , Xiaohui Fan , Wei Jeat Hon , David Raithel , Patrick Tisserand , Sameul Lai

The quasar Q1208+1011 (z_{em}=3.8) is the second highest redshift double quasar ever detected. Several indications point toward it being a gravitational lensed system, although a definitive proof is still lacking. We present new evidence of…

Astrophysics · Physics 2009-10-30 E. Giallongo , A. Fontana , S. Cristiani , S. D'Odorico

We report the discovery of a radio-loud flat-spectrum QSO at z=5.47 with properties similar to those of the EGRET gamma-ray blazars. This source is the brightest radio QSO at z>5, with a pc-scale radio jet and a black hole mass estimate…

Astrophysics · Physics 2009-11-10 Roger W. Romani , David Sowards-Emmerd , Lincoln Greenhill , Peter Michelson

We present the discovery of a gravitationally lensed dust-reddened QSO at $z=2.517$ discovered in a survey for red QSOs by infrared selection. $Hubble~Space~Telescope$ imaging in the WFC3/IR F160W and F125W filters reveals a quadruply…

Astrophysics of Galaxies · Physics 2018-07-17 E. Glikman , C. E. Rusu , S. G. Djorgovski , M. J. Graham , D. Stern , T. Urrutia , M. Lacy , J. M. O'Meara

Gravitational lensing sometimes dominates the observed properties of apparently very bright objects. We present morphological properties in the high-resolution (FWHM $\sim0.''15$) Atacama Large Millimeter/submillimeter Array (ALMA) 1-mm map…

Astrophysics of Galaxies · Physics 2020-03-11 Seiji Fujimoto , Masamune Oguri , Tohru Nagao , Takuma Izumi , Masami Ouchi

Distant luminous quasars provide important information on the growth of the first supermassive black holes, their host galaxies and the epoch of reionization. The identification of quasars is usually performed through detection of their…

Astrophysics of Galaxies · Physics 2017-06-20 Ekaterina Koptelova , Chorng-Yuan Hwang , Po-Chieh Yu , Wen-Ping Chen , Jhen-Kuei Guo

Quasars are the most luminous non-transient objects known and as a result they enable studies of the Universe at the earliest cosmic epochs. Despite extensive efforts, however, the quasar ULAS J1120+0641 at z=7.09 has remained the only one…

We aim to illustrate the potentiality of the Advanced Large, Homogeneous Area, Medium-Band Redshift Astronomical (ALHAMBRA) survey to investigate the high redshift universe through the detection of quasi stellar objects (QSOs) at redshifts…

We present observations of SDSSp J104433.04--012502.2, a luminous quasar at z=5.80 discovered from Sloan Digital Sky Survey (SDSS) multicolor imaging data. This object was selected as an i'-band dropout object, with i*=21.8 +/- 0.2, z*=19.2…

Measurements of QSO clustering in the SDSS show that $\mathrm{z}>4$ QSOs are some of the most highly biased objects in the universe. Their large correlation lengths of $r_0 \sim 20h^{-1}$Mpc are comparable to the most massive clusters of…

Astrophysics of Galaxies · Physics 2015-06-22 Scott M. Adams , Paul Martini , Kevin V. Croxall , Roderik A. Overzier , John D. Silverman

From 2011 to 2021, LAMOST has released a total of 76,167 quasar data. We try to search for gravitationally lensed QSOs by limiting coordinate differences and redshift differences of these QSOs. The name, brightness, spectrum, photometry and…

Astrophysics of Galaxies · Physics 2023-08-29 Y. H. Chen , M. Y. Tang , H. Shu , H. Tu

We present the discovery of a gravitationally lensed dust-reddened QSO at z = 2.517, identified in a survey for QSOs by infrared selection. Hubble Space Telescope imaging reveals a quadruply lensed system in a cusp configuration, with a…

Strong gravitational lensing provides a powerful probe of the physical properties of quasars and their host galaxies. A high fraction of the most luminous high-redshift quasars was predicted to be lensed due to magnification bias. However,…

We report the discovery of an ultra-luminous quasar J030642.51+185315.8 (hereafter J0306+1853) at redshift 5.363, which hosts a super-massive black hole (SMBH) with $M_{BH} = (1.07 \pm 0.27) \times10^{10}~M_\odot$. With an absolute…

2MASX J04035024-0239275 is a bright red elliptical galaxy at redshift 0.0661 that presents two extended sources at 2\arcsec~to the north-east and 1\arcsec~to the south-west. The sizes and surface brightnesses of the two blue sources are…

Cosmology and Nongalactic Astrophysics · Physics 2018-06-13 Lluís Galbany , Thomas E. Collett , Jairo Méndez-Abreu , Sebastián F. Sánchez , Joseph P. Anderson , Hanindyo Kuncarayakti

The study of absorptions along the lines of sight to bright high-$z$ QSOs is an invaluable cosmological tool that provides a wealth of information on the inter-/circum-galactic medium, Dark Matter, primordial elements, reionization,…

Instrumentation and Methods for Astrophysics · Physics 2020-01-08 Calderone G. , Boutsia K. , Cristiani S. , Grazian A. , Amorin R. , D'Odorico V. , Cupani G. , Fontanot F. , Salvato M

We present sensitive near--infrared VLT ISAAC spectroscopic observations of the z=6.08 quasar SDSS J030331.40-001912.9. This QSO is more than a magnitude fainter than other QSOs at z~6 for which NIR spectroscopy has been obtained to date…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 J. D. Kurk , F. Walter , X. Fan , L. Jiang , S. Jester , H. -W. Rix , D. A. Riechers
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